Figure 4.
Halo GV optical density measurement as a function of hydrostatic pressure (N=3 independent preparations). The error bars are standard error. The data was fit to a Boltzmann sigmoid fit of the form f(p) = (1+e(p − pc)/Δp )−1 with Δp = 8 kPa and an average midpoint of collapse pc= 64 kPa (R2>0.998).
